Venera 13 and Venera 14: Sedimentary Rocks on Venus?
- 1 July 1983
- journal article
- other
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 221 (4605), 57-59
- https://doi.org/10.1126/science.221.4605.57
Abstract
Venera 13 and Venera 14 transmitted almost complete panoramic views of their landing sites. Analyses of the photographs show the presence of rock formations undergoing geomorphic degradation. The formations display ripple marks, thin layering, differential erosion, and curvilinear fracturings. Some of them are interpreted as lithified clastic sediments. The lithification could have taken place at depth or at the surface, resulting in a type of duricrust. The origin of the sediments is unknown but could be aeolian, volcanic, or related to impacts or to turbidity currents.Keywords
This publication has 6 references indexed in Scilit:
- Venus Was Wet: A Measurement of the Ratio of Deuterium to HydrogenScience, 1982
- Geomorphic Degradations on the Surface of Venus: An Analysis of Venera 9 and Venera 10 DataScience, 1977
- The surface of Venus as revealed by Soviet Venera 9 and 10GSA Bulletin, 1977
- Windblown Dust on Earth, Mars and VenusJournal of the Atmospheric Sciences, 1976
- Dust on VenusJournal of the Atmospheric Sciences, 1975
- Aeolian regime of the surface of VenusAstrophysics and Space Science, 1970